Particle Theory GroupZoltan Ligeti

(ligeti@berkeley.edu)

March 16, 2018

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Who we are

Christian Bauer Zoltan Ligeti Michele Papucci Kathryn Zurek

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Who we really are: BCTP

Christian Bauer Zoltan Ligeti Michele Papucci Kathryn Zurek

Lawrence Hall Hitoshi Murayama Yasunori Nomura Surjeet Rajendran

Mina Aganagic Raphael Bousso Ori Ganor Petr Hořava

+ postdocs

+ students

+ visitors

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BCTP postdocs

Bao Dror Fedderke Harigaya

Galakhov Grabowska Knapen Kos

Lou Moult Ramani Remmen

• One of the largest and best groups of postdocs in the country, many work with graduate studentsp.2 p.2

The particle theory side

Experiments|

QCD, collider physics, Higgs:Bauer, Ligeti, Papucci, Zurek, Murayama

BSM Phenomenology:Ligeti, Papucci, Zurek,Hall, MurayamaNomura, Rajendran

Model building:Papucci, Zurek,Hall, MurayamaNomura, Rajendran

Flavor physics:Bauer, Ligeti, Papucci

Dark matter, cosmic rays:Papucci, Zurek, NomuraHall, Murayama, Rajendran

Neutrinos:Zurek, Murayama

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What and how...

• Those of you who attended the BCTP open house yesterday heard already a lot• We are leaders in many areas of particle theory• Research interests evolve depending on what are the most relevant questions to

address at the moment — “What’s most exciting?”

• Each of us has his/her own way to approach problems — Important for you to beexposed to many different ways of doing physics in a large and diverse group

• Students and postdocs are free to collaborate with anyone (encouraged!)(Most doors open, exciting & lively discussions all the time, yearly retreats at Lake Tahoe)

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Some research interests (random order)

Develop effective field theories, apply to various problems (flavor, jets, DM, cosmology, ...)

Precision SM calculations, Monte Carlo methods / tools

Collider physics: SM measurements and BSM searches

Flavor physics, CP violation, low-energy searches for NP

Electroweak scale BSM model building / Higgs phenomenology

Dark matter model building, new techniqes for DM detection

Dark matter searches (direct detection + indirectly with particle astrophysics)

Proposals for new detectors, new analysis techniques

Early universe particle cosmology

Neutrino physics, leptogenesis models

Inflationary models

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Connections to experiments

• LBNL has the strongest university connection among the national labs(more so than, e.g., SLAC–Stanford)

• In BCTP we operate as a single group (Mon/Tue on campus, Wed/Thu at LBL,seminars split between campus and LBL accordingly)

• Closeness to extensive experimental programs, many interactions(joint seminars & workshops, etc.)

• Particle theory graduate students exposed to broad spectrum of experimentalresearch at LBL, can become important in shaping careers

• Experimental graduate students have easy access to the theory group for adviceon theoretical aspects of their research (just walk down the corridor or catchsomeone at the espresso machine...)

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Theory – experiment connections

• Logistics at LBL makes it extremely easy for theorists and experimentalists tointeract on a daily basis

• Regular ATLAS–Theory lunches (informal talks→ discussions, collaborations)• Many of us provide theoretical advice to experiments:

ATLAS, DM detection, neutrinos, flavor physics, PDG

Even propose new experiments / techniques

• In the past some of these resulted in direct involve-ment in experiments (Cahn, Hinchliffe, Murayama)

Hitoshi taking shifts in KamLAND −→

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My personal views

• After Higgs discovery, situation may resemble around 1900 — we don’t under-stand a “few” things (a lot left for you!) ⇒ may see revolutions, but no guarantees(Michelson 1894: “... it seems probable that most of the grand underlying principles have been firmly established ...”)

Dark energy — cosmological constant?Dark matter — vast parameter space; only interact gravitationally?Baryon asymmetry — originates at very high scales?Neutrino mass — Majorana or Dirac? (lepton number viol.?)Strong CP problem — axion?Flavor parameters and hierarchies — very high scales?

Leave no stone unturned — explore fully what technologies allow

• Move the lamp post: e.g., new LHC searches, new DM or axion param’ space• Search better under the lamp post: e.g., Higgs couplings, B decays & CP violation• Historically, the combination of both approaches proved most fruitful

Most of us work on both type of questions

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And an apology...

• In past years we always had a breakout with theory postdocs, parallel to lab tours

• See http://www-theory.lbl.gov/ and http://ctp.berkeley.edu/All of us (present or not) would be happy to talk to you!

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http://www-theory.lbl.gov/http://ctp.berkeley.edu/

Thank you, and...

Congr

atulati

ons! ! !